Dataciencia

Colección SciELO Chile

HD 101584: circumstellar characteristics and evolutionary status

Indexado

WoS	WOS:000462115700001
Scopus	SCOPUS_ID:85063742728

DOI

10.1051/0004-6361/201834897

Año

2019

Tipo

artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras

Abstract

Conclusions. We provide good evidence that the binary system HD 101584 is in a post-common-envelope-evolution phase, that ended before a stellar merger. Isotope ratios combined with stellar mass estimates suggest that the primary star's evolution was terminated already on the first red giant branch (RGB). Most of the energy required to drive the outflowing gas was probably released when material fell towards the companion.

Revista

Revista	ISSN
Astronomy & Astrophysics	0004-6361

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Disciplinas de Investigación

WOS
Astronomy & Astrophysics

Scopus
Sin Disciplinas

SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional

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Autores - Afiliación

Ord.	Autor	Género	Institución - País
1	Olofsson, H.	Hombre	Chalmers Univ Technol - Suecia Chalmers University of Technology, Onsala Space Observatory - Suecia Onsala Space Observatory - Suecia
2	Khouri, T.	-	Chalmers Univ Technol - Suecia Chalmers University of Technology, Onsala Space Observatory - Suecia Onsala Space Observatory - Suecia
3	Maereker, M.	-	Chalmers Univ Technol - Suecia
3	Maercker, M.	-	Chalmers University of Technology, Onsala Space Observatory - Suecia
4	Ségransan, Damien	Hombre	Chalmers Univ Technol - Suecia Chalmers University of Technology, Onsala Space Observatory - Suecia Onsala Space Observatory - Suecia
5	Doan, L.	-	UPPSALA UNIV - Suecia Uppsala Universitet - Suecia
6	Tafoya, D.	Hombre	Natl Astron Observ Japan - Japón National Institutes of Natural Sciences - National Astronomical Observatory of Japan - Japón
7	Vlemmings, W. H. T.	Hombre	Chalmers Univ Technol - Suecia Chalmers University of Technology, Onsala Space Observatory - Suecia Onsala Space Observatory - Suecia
8	Humphreys, E. M. L.	-	ESO - Alemania
9	Lindqvist, Michael	Hombre	Chalmers Univ Technol - Suecia Chalmers University of Technology, Onsala Space Observatory - Suecia Onsala Space Observatory - Suecia
10	Nyman, L.	-	ESO - Chile
11	Ramstedt, S.	-	UPPSALA UNIV - Suecia

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Origen de Citas Identificadas

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 5.88 %
Citas No-identificadas: 94.12 %

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Citas identificadas: Las citas provienen de documentos incluidos en la base de datos de DATACIENCIA

Citas Identificadas: 5.88 %
Citas No-identificadas: 94.12 %

Financiamiento

Fuente
National Science Foundation
European Research Council
Swedish Research Council
ERC
National Aeronautics and Space Administration
Seventh Framework Programme
VetenskapsrÃ¥det
ASIAA
National Rehabilitation Center
Vetenskapsradet
University of California, Los Angeles
European School of Oncology
Alberta Livestock and Meat Agency
Korea Astronomy and Space Science Institute
National Institutes of Natural Sciences
California Institute of Technology
Jet Propulsion Laboratory
Jet Propulsion Laboratory/California Institute of Technology

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos

Agradecimiento
H.O. and W.V. acknowledge support from the Swedish Research Council. W.V. acknowledges support from the ERC through consolidator grant 614264. This paper makes use of the following ALMA data: ADS/JAO. ALMA#2012.1.00248.S and #2015.1.00078.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan) and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. This paper makes use of the following APEX data: O-093.F-9307, O-096.F-9303, O-098.F-9314, O-099.F-9310, O-0100.F-9302, O-0101.F-9302, and O-0102.F-9402A (SEPIA Band 9 Science Verification data). The Atacama Pathfinder EXperiment (APEX) is a collaboration between the Max-Planck-Institut fur Radioastronomie, the European Southern Observatory, and the Onsala Space Observatory. This paper has also made use of the NASA/IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration, and data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. Frederic Schuller is gratefully acknowledged for help with the reduction of the ArTeMiS data. Finally, we are grateful to the anonymous referee who provided a very constructive report.
Acknowledgements. H.O. and W.V. acknowledge support from the Swedish Research Council. W.V. acknowledges support from the ERC through consolidator grant 614264. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2012.1.00248.S and #2015.1.00078.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan) and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. This paper makes use of the following APEX data: O-093.F-9307, O-096.F-9303, O-098.F-9314, O-099.F-9310, O-0100.F-9302, O-0101.F-9302, and O-0102.F-9402A (SEPIA Band 9 Science Verification data). The Atacama Pathfinder EXperiment (APEX) is a collaboration between the Max-Planck-Institut für Radioastronomie, the European Southern Observatory, and the Onsala Space Observatory. This paper has also made use of the NASA/ IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration, and data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. Frederic Schüller is gratefully acknowledged for help with the reduction of the ArTeMiS data. Finally, we are grateful to the anonymous referee who provided a very constructive report.

Agradecimiento

H.O. and W.V. acknowledge support from the Swedish Research Council. W.V. acknowledges support from the ERC through consolidator grant 614264. This paper makes use of the following ALMA data: ADS/JAO. ALMA#2012.1.00248.S and #2015.1.00078.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan) and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. This paper makes use of the following APEX data: O-093.F-9307, O-096.F-9303, O-098.F-9314, O-099.F-9310, O-0100.F-9302, O-0101.F-9302, and O-0102.F-9402A (SEPIA Band 9 Science Verification data). The Atacama Pathfinder EXperiment (APEX) is a collaboration between the Max-Planck-Institut fur Radioastronomie, the European Southern Observatory, and the Onsala Space Observatory. This paper has also made use of the NASA/IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration, and data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. Frederic Schuller is gratefully acknowledged for help with the reduction of the ArTeMiS data. Finally, we are grateful to the anonymous referee who provided a very constructive report.

Acknowledgements. H.O. and W.V. acknowledge support from the Swedish Research Council. W.V. acknowledges support from the ERC through consolidator grant 614264. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2012.1.00248.S and #2015.1.00078.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan) and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. This paper makes use of the following APEX data: O-093.F-9307, O-096.F-9303, O-098.F-9314, O-099.F-9310, O-0100.F-9302, O-0101.F-9302, and O-0102.F-9402A (SEPIA Band 9 Science Verification data). The Atacama Pathfinder EXperiment (APEX) is a collaboration between the Max-Planck-Institut für Radioastronomie, the European Southern Observatory, and the Onsala Space Observatory. This paper has also made use of the NASA/ IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration, and data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. Frederic Schüller is gratefully acknowledged for help with the reduction of the ArTeMiS data. Finally, we are grateful to the anonymous referee who provided a very constructive report.

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Abstract

Revista

Métricas Externas

Disciplinas de Investigación

Colaboración Institucional

Autores - Afiliación

Origen de Citas Identificadas

Financiamiento

Agradecimientos

Departamento Gestión de Conocimiento, Monitoreo y Prospección